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Titlebook: Magnetic Fields of Celestial Bodies; Ye Shi-Hui Book 1994 Springer Science+Business Media Dordrecht 1994 Magnetic field.Planet.Solar Syste

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41#
發(fā)表于 2025-3-28 15:56:07 | 只看該作者
Ye Shi-Huipensable for moral and social behaviour are discovered and the brains of psychopaths and criminals - the classical anti-heroes of morality - are scanned with curiosity, even enthusiasm...How revolutionary this current research might be, the quest for a localisable ethical centre or moral organ is fa
42#
發(fā)表于 2025-3-28 20:05:33 | 只看該作者
Ye Shi-Huiwith a description of the types of arguments and modifiers allowed in these constructions (namely, adjectives, prepositional phrases (PPs), and genitive pronouns). The analysis of these data enables me to determine the basic design of Spanish nominal constructions and to explain the structural relat
43#
發(fā)表于 2025-3-29 02:37:48 | 只看該作者
44#
發(fā)表于 2025-3-29 04:18:07 | 只看該作者
Introduction,t the Sun might possess a magnetic field like that of the Earth. His speculation was based upon the similarity of the fine coronal plumes near the polar regions, photographed during solar total eclipses, to the field lines of a magnetized sphere. But the first formal and reliable evidence of the exi
45#
發(fā)表于 2025-3-29 08:31:53 | 只看該作者
46#
發(fā)表于 2025-3-29 14:03:45 | 只看該作者
Techniques for the Measurement of Magnetic Fields of Celestial Bodies, chapter we proceed to discuss some technical questions. We are aware of the fact that there are many kinds of instruments specially designed and constructed for magnetic measurements of heavenly objects (in particular, the Sun) and that most of them are quite sophisticated in their optical layout,
47#
發(fā)表于 2025-3-29 17:53:56 | 只看該作者
48#
發(fā)表于 2025-3-29 22:09:27 | 只看該作者
Background and Local Magnetic Fields on the Solar Surface,netism. Magnetic lines of force pervade various parts of the solar disk and every layer of the solar atmosphere. Strictly speaking, there is no region which is a real vacuum for magnetism. Starting here, we shall devote three chapters to the solar magnetic fields outside spots. Roughly speaking, thi
49#
發(fā)表于 2025-3-30 02:27:31 | 只看該作者
Magnetic Fields of the Solar Atmosphere,f only about 500 km. Above it is the chromosphere with a thickness of approximately 20,000 km. The outmost part is the corona, which has a scope of several to ten more solar radii. Its shape is not fixed and varies with the phase of the solar activity cycle. The magnetic field pervades the whole sol
50#
發(fā)表于 2025-3-30 05:19:49 | 只看該作者
The General Magnetic Field of the Sun,ffect the structure and evolution of the Sun. Second, the physical interpretation of the solar activity cycle. requires that the entire solar globe, especially the high-latitude regions, possesses magnetism. Third, as will be described in the next chapter, the solar wind brings the magnetic field of
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